| discov_num |
notes |
refcode |
| SHJ 243 |
36 Oph = A Oph. AB = HDO 144. Proper motion -480 -1142. A premature |
|
|
orbit has been computed. A may be a spectroscopic binary. |
|
|
Three orbit solutions by Irwin et al. (1996); the shortest-period |
Irw1996 |
|
orbit is marginally preferable. |
|
|
VLTI uniform disk diameter of A: 1.253 +/- 0.025 mas, |
LTI2009 |
|
VLTI limb-darkened disk diameter of A: 1.282 +/- 0.026 mas, |
|
|
R = 0.817 +/- 0.016 \rsun, Teff = 4843 +/- 134 K. |
|
|
AC: NLTT 44415/44446 |
Chm2004 |
|
AC: SHY 87. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
|
C component = CD-26 12036 (mag. 6.34, 700", K5V), proper motion |
|
|
-481 -1134. C has common proper motion. |
|
|
The original AC and BC components in the BDS and ADS were changed |
|
|
to AD and BD in the IDS to accommodate the discovery by Luyten |
Luy1941 |
|
(= LDS 588) assigned AC. This component assignment has been |
|
|
maintained. However, the BC measures from the BDS were erroneously |
|
|
assigned to the AD component in the IDS and two AC measures were |
|
|
assigned to the BD. This has been corrected, as have errors made |
|
|
in the IDS in the measures of South and Jacob of the AD and BD |
S__1824 |
|
components. PM of D +003+026. |
Jc_1848b |
|
AD: Optical pair, based on study of relative motion of the components |
|
|
using the method of apparent motion parameters. |
Kiy2008 |
|
AE: Rectilinear solution by Mason & Hartkopf (2016). |
Msn2016a |
|
BD: Rectilinear solution by Friedman et al. (2011). |
USN2011a |
| refcode |
metd |
author |
reference |
| Chm2004 |
E - |
Chaname, J. & Gould, A. |
2004ApJ...601..289C |
| Chm2004 |
|
ApJ 601, 289, 2004 |
|
| Chm2004 |
|
(Photometry, coordinates, and astrometry from rNLTT. Astrometry from early |
|
| Chm2004 |
|
versions of 2MASS and UCAC, with date given only as "circa 2000". Measures |
|
| Chm2004 |
|
identical to discovery observations - predominantly close pairs - were assumed |
|
| Chm2004 |
|
not new observations, so not included in WDS. Similar concerns when primary and |
|
| Chm2004 |
|
secondary magnitudes or proper motions were the same.) |
|
| Irw1996 |
orb - |
Irwin, A.W., Yang, S.L.S., & Walker, G.A.H. |
1996PASP..108..580I |
| Irw1996 |
|
PASP 108, 580, 1996 |
|
| Jc_1848b |
Ma j |
Jacob, W.S. |
1854MadOO....8b...1 |
| Jc_1848b |
|
Madras Obs. 8, 1848-1852 Appendix |
|
| Kiy2008 |
- |
Kiyaeva, O.V., Kiselev, A.A. & Izmailov, I.S. |
2008SvAL...32..405K |
| Kiy2008 |
|
SvAL 34, 405, 2008 |
|
| LTI2009 |
not j |
Demory, B.-O., Segransan, D., Forveille, T., Queloz, D., Beuzit, J.-L., Delfosse, |
2009A&A...505..205D |
| LTI2009 |
|
X., Di Folco, E., Kervella, P., Le Bouquin, J.-B., Perrier, C., Benisty, M., |
. |
| LTI2009 |
|
Duvert, G., Hofmann, K.-H., Lopez, B. & Petrov, R. |
. |
| LTI2009 |
|
A&A 505, 205, 2009 |
. |
| Luy1941 |
Po - |
Luyten, W.J. |
1941POMin...3....1L |
| Luy1941 |
|
Pub. Univ. Minnesota Obs. 3, #3, 1941 |
|
| Luy1941 |
|
(CPM pairs found by comparison of Bruce proper motion plates. First and second |
|
| Luy1941 |
|
plates epochs were 1898-1904 and 1928-1936, so a default mean date of 1920 was |
|
| Luy1941 |
|
assigned to all measures.) |
|
| Msn2016a |
lin - |
Mason, B.D. & Hartkopf, W.I. |
2016IAUDS.189....1M |
| Msn2016a |
|
Inf. Circ. 189, 1, 2016 |
|
| Shy2011 |
- |
Shaya, E.J. & Olling, R. |
2011ApJS..192....2S |
| Shy2011 |
|
ApJS 192, 2, 2011 |
|
| Shy2011 |
|
(Statistical analysis of probability that wide Hipparcos pairs are physical. Pairs |
|
| Shy2011 |
|
added to WDS only if probability 90% or greater.) |
|
| USN2011a |
lin - |
Friedman, E.A., Mason, B.D., & Hartkopf, W.I. |
2011IAUDS.175....1F |
| USN2011a |
|
Inf. Circ. 175, 1, 2011 |
|
